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Inferring the delay time distribution of type Ia supernovae with CAALAM I: SED modelling choices and their effect on the delay time distribution
A delay time distribution (DTD) quantifies the lag between progenitor formation and the subsequent explosive event. The DTD for a sample of Type Ia supernovae (SNe Ia) from a survey can be modelled through relative rates and the star formation histories (SFH) of all individual galaxies. Modern wide-
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